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1دورية أكاديمية
المؤلفون: Wielgórski, Piotr, Pietrzyński, Grzegorz, Pilecki, Bogumił, Gieren, Wolfgang, Zgirski, Bartłomiej, Górski, Marek, Hajdu, Gergely, Narloch, Weronika, Karczmarek, Paulina, Smolec, Radosław, Kervella, Pierre, Storm, Jesper, Gallenne, Alexandre, Breuval, Louise, Lewis, Megan, Kałuszyński, Mikołaj, Graczyk, Dariusz, Pych, Wojciech, Suchomska, Ksenia, Taormina, Mónica, Rojas Garcia, Gonzalo, Kotek, Aleksandra, Chini, Rolf, Pozo Nũnez, Francisco, Noroozi, Sadegh, Sobrino Figaredo, Catalina, Haas, Martin, Hodapp, Klaus, Mikołajczyk, Przemysław, Kotysz, Krzysztof, Moździerski, Dawid, Kołaczek-Szymański, Piotr
المساهمون: Copernicus Astronomical Center of the Polish Academy of Sciences (CAMK), Polska Akademia Nauk = Polish Academy of Sciences = Académie polonaise des sciences (PAN), Universidad de Concepción = University of Concepción Chile (UdeC), Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), University of Wrocław Poland (UWr), P.W. gratefully acknowledges financial support from the Polish National Science Center grant PRELUDIUM 2018/31/ N/ST9/02742. The research leading to these results has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreements No. 695099 and No. 951549). Support from DIR/WK/2018/12 grant of the Polish Ministry of Science and Higher Education and the Polish National Science Center grants MAESTRO 2017/26/A/ST9/ 00446 and BEETHOVEN 2018/31/G/ST9/03050 is also acknowledged. W.G. and G.P. gratefully acknowledge financial support for this work from the BASAL Centro de Astrofisica y Tecnologias Afines (CATA) AFB-170002. B.P. gratefully acknowledges support from the Polish National Science Center grant SONATA BIS 2020/38/E/ST9/00486. R.S. gratefully acknowledges support from the Polish National Science Center grant SONATA BIS 2018/30/E/ST9/00598. A.G acknowledges support from the ALMA-ANID fund No. ASTRO20-0059. F.P. gratefully acknowledges the generous and invaluable support of the Klaus Tschira Foundation. Based on data collected under the ESO/CAMK PAN—USB agreement at the ESO Paranal Observatory. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.intTest/ gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaiaTest/ dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This research has made use of the SIMBAD database, operated at Centre de Données astronomiques de Strasbourg, France., European Project: 730997,EUROCHAMP2020(2020)
المصدر: ISSN: 0004-637X.
مصطلحات موضوعية: Type II Cepheid variable stars, Pulsating variable stars, Large Magellanic Cloud, Milky Way Galaxy, Distance indicators, Galaxy distances, Stellar distance, Population II Cepheid variable stars, Population II stars, [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2112.12122; info:eu-repo/grantAgreement//730997/EU/European Union’s Horizon 2020 research and innovation programme under grant agreement/EUROCHAMP2020; hal-03667347; https://u-paris.hal.science/hal-03667347Test; https://u-paris.hal.science/hal-03667347/documentTest; https://u-paris.hal.science/hal-03667347/file/Wielg%C3%B3rski_Pietrzy%C5%84ski_Pilecki%20et%20al._Article_An%20Absolute._2022.pdfTest; ARXIV: 2112.12122
الإتاحة: https://doi.org/10.3847/1538-4357/ac470cTest
https://u-paris.hal.science/hal-03667347Test
https://u-paris.hal.science/hal-03667347/documentTest
https://u-paris.hal.science/hal-03667347/file/Wielg%C3%B3rski_Pietrzy%C5%84ski_Pilecki%20et%20al._Article_An%20Absolute._2022.pdfTest -
2مؤتمر
المؤلفون: Wielgorski, Piotr1 pwielgor@camk.edu.pl, Pietrzynski, Grzegorz1,2, Gieren, Wolfgang2,3
المصدر: EPJ Web of Conferences. 2017, Vol. 152 Issue 32592742, p1-2. 2p.
مصطلحات موضوعية: *SMALL magellanic cloud, *STELLAR luminosity function, *CEPHEIDS, *EXTRAGALACTIC distances, *LARGE magellanic cloud, *NEAR infrared spectroscopy